Convective boundary mixing in a post-He core burning massive star model
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DOI: 10.1093/mnras/sty3415
Abstract: Convective boundary mixing (CBM) in the advanced evolutionary stages of massive stars is not well understood. Structural changes caused by convection have an impact on the evolution as well as the subsequent supernova, or lack… read more here.
Keywords: cbm; odot mathrm; mathrm odot; model ... See more keywords